A known technique for solving (systems of) differential equations is based on the Laplace transformation. This is a linear mapping between certain vector spaces of functions. Here we discuss the definition of the Laplace transform and its linearity. Later we will discuss the most important calculation rules and applications to solving (systems of) differential equations.
The Laplace transform of a function defined on is the function , for sufficiently large defined by
The Laplace transformation is the mapping which assigns to the Laplace transform of .
The Laplace transform of the constant function is
that is defined on and so on each interval of form where .
The Laplace transform thus assigns to a function on the interval (for which the indicated definite integral exists) a function on an interval . It is thus a mapping from the vector space of real-valued functions on (for which the indicated definite integral exists) to the set of all the functions which are defined on an interval of the shape .
The argument of the function is often denoted by in order to emphasize its association with time; this is related to the restriction . In the function rule of the Laplace-transform the variable is typically used as an argument. The Laplace transform then supplies a transition from the time domain (-domain for short) to the frequency domain (-domain for short).
Often, instead of the notation or is used. We avoid using the braces and , since their meaning is the usual one for brackets. If is a compound expression, we also write in order to make clear what the argument of is. Note that in the Laplace transform has priority over application to : it would be clearer if we wrote , but we try and reduce the use of brackets so as to keep the expressions legible.
Sometimes, we use the notation for .
The Laplace transform is not defined for every function. But if exists for a certain value , then it exists for all . After all, the function of rapidly approaches if goes to ; the larger , the faster the approximation.
The Laplace transform is hardly ever calculated by use of the integral definition. Instead, calculation rules are used. The first such rule is linearity:
Suppose that and are continuous functions with the property that and exist. If , are real numbers, then
In other words, the Laplacian operator is a linear map from the vector space of all continuous real functions for which the integral exists, to the vector space of all real functions which are defined on an interval of the shape for a real number .
Further calculation rules:
Let and be real numbers with and let be a natural number.
Special cases:
As we will be able to see in the example below, the Laplace transforms of the trigonometic functions sine and cosine are given by
The rule for the time scaling gives
The rule for the derivative in the frequency domain gives
The rule for a frequency shift gives
Time scaling:
Frequency shift:
Derivative in frequency domain: we first prove the case ; here we use the fact that under the given circumstances, differentiation with respect to and integration with respect to may be interchanged changed
By induction on we derive the general case, , from this:
The first two special cases follow from the rule for the derivative in the frequency domain by taking and , respectively. The third special case follows from the previous special case by application of linearity and a frequency shift.
Here are some examples:
Compute the Laplace transform of the function on defined by
Give your answer as a function in the variable for .
By use of the definition of Laplace transform we find
By use of linearity we can find the Laplace transform more rapidly: